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  3. Energy transfers
  4. Radiation

Energy transfers · Process

Radiation

Conduction needs particles touching. Convection needs a fluid that can move. Between here and the Sun there is neither — and yet you can feel sunlight on your face.

Start here

Conduction and convection both fail here.

Conduction needs particles touching. Convection needs a fluid that can move. Between here and the Sun there is neither — space is empty. And yet you can feel sunlight on your face, and it arrives eight minutes after it leaves.

Commit to how it crosses.

Radiation is the third and last of the routes, and it is the odd one out twice over: it needs no particles, and it travels in straight lines in every direction rather than following the material. Everything above absolute zero emits it — you, this page, a block of ice — and what changes with temperature is only how much.

Three routes · take them away one at a time

Which routes survive?

Move the detector and take the air away. Watch which of the three routes can still deliver anything — and note which one never stops working.

Conduction

Convection

Radiation

All the routes that can work are working. Warm air rises straight into the detector, and radiation arrives as well — which is why this is the situation that convinces people heat only goes up.

Key fact

Infrared radiation is an electromagnetic wave. It needs no particles at all, crosses a vacuum, and is emitted by every object — more from hotter surfaces, and more from matt black ones than from shiny silver ones.

The word “radiation” · where is the boundary?

Six kinds of radiation. Three of them are harmless.

Everything here is radiation. Sort each one, then find the line — it is not where most people put it.

Infrared from a radiator

Visible light from a lamp

Radio waves from a phone mast

Ultraviolet from the Sun

X-rays in a hospital

Gamma rays from a nuclear source

Think again

“Heat rises, so heating always travels upwards.”

What rises is warm air, because it is less dense than the cold air around it and floats on it. That is convection, and it genuinely does go upwards. But it is one route out of three, and the other two ignore gravity entirely.

Radiation travels in straight lines in every direction at once — up, down, sideways. Stand beside a bonfire and one side of you is warm; lie under a patio heater and the warmth comes down. Conduction is equally indifferent: hold a metal rod pointing downwards into a flame and the far end still gets hot.

“Heat rises” is a fact about air, stated as if it were a law about energy. Say “warm air rises” and the confusion disappears.

“Only hot things give out infrared radiation.”

Everything above absolute zero emits it, including you, this page and a block of ice. What changes with temperature is how much: a hotter surface emits far more, and at shorter wavelengths. A thermal camera pointed at a snowy field still sees a picture, because the snow is radiating too — it is simply radiating less than everything around it.

Mastery ladder

Not started yet.

Rungs 3 and 4 you mark yourself.

Rung 1 · Recall

Which method of energy transfer does not need any material to travel through?

Rung 2 · The one that catches people

You stand to the side of a bonfire, level with the flames, and feel warmth on your face. Which transfer is reaching you?

Rung 3 · Explain

Explain how energy from the Sun reaches the Earth, and why the other two methods of transfer cannot be responsible.

Rung 4 · Take it somewhere new

A news report describes a new patio heater as “using radiation to warm your garden” and a reader complains it sounds unsafe. Write a reply that is accurate about both the physics and the risk.

Key note

Radiation needs no material and travels in every direction, which is why it is the only route across a vacuum and why warmth does not only go upwards. Everything emits it. Only the high-energy end of the family — ultraviolet and beyond — can do harm.

Going further

If everything emits radiation, why is the night sky dark? The question is older than it looks — it is called Olbers' paradox, and it goes like this: in an infinitely old, infinitely large universe full of stars, every line of sight would eventually end on a star, and the whole sky would blaze as brightly as the Sun. It does not. The resolution is that the universe is neither infinitely old nor unchanging: there has not been enough time for light from the most distant parts to reach us, and the expansion of space has stretched what does arrive to wavelengths far below visible. The dark sky is evidence that the universe had a beginning — which is a great deal to get from looking up.

Before this lesson

At GCSE this becomes

  • The electromagnetic spectrum in full, with wavelength and frequency attached to each band, and absorption and emission treated as a rate.

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